General relativity and Newton's laws

In summary, the conversation discusses the gravitational force acting on a particle of mass m on the surface of a sphere with a mass of 10^52 kg and a radius of 10^24 meters. The question is whether this force is given by the Newtonian value or if general relativity is required for a sensible result. The conversation also touches on the concept of gravitons and the relationship between mass and gravity in general relativity.
  • #1
kurious
641
0
Is the gravitational force acting on a particle of mass m, on the
surface of a sphere of radius 10^24 metres and with a mass of
10^52 kg given by G x10^52 m / (10^24 ) ^ 1/2 - the Newtonian value - or is the mass density high enough for general relativity to be required to get a
sensible result?
 
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  • #2
kurious said:
Is the gravitational force acting on a particle of mass m, on the
surface of a sphere of radius 10^24 metres and with a mass of
10^52 kg given by G x10^52 m / (10^24 ) ^ 1/2 - the Newtonian value - or is the mass density high enough for general relativity to be required to get a
sensible result?

r is squared, not square rooted. In general relativity The law of motion can be written [tex]F^\lambda = m(\frac{dU^\lambda }{d\tau }) + m\Gamma ^{\lambda }_{\mu }_{\nu }U^{\mu }U^{\nu }[/tex].
The real force on your test mass is the normal force holding it up and is expressed as the four vector on the left hand side of the equation. The last expression on the right can be called the gravitational force, but is only an inertial force which are sometimes called fictitious forces. What I think you really intend to compare is the prediction from Newtonian mechanics for the weight measured on a scale Vs the prediction for the measurement from general relativity. What the scale really reads is the reaction force on it associated to the real normal force up on the test mass. The readout for the general relativisitc prediction would be given from equation 10.2.1 at
http://www.geocities.com/zcphysicsms/chap10.htm#BM10_2
[tex]F'_{felt} = \frac{GMm/r^{2}}{\sqrt{1 - \frac{2GM}{rc^2}}}[/tex]
 
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  • #3
Apparently, a mass can't be held still over the event horizon of a black hole, so the mass I was talking about would have to be in motion on the surface of the sphere.
If gravitons exist would they have to account for the "felt" force or F lambda?
 
  • #4
kurious said:
Apparently, a mass can't be held still over the event horizon of a black hole, so the mass I was talking about would have to be in motion on the surface of the sphere.
If gravitons exist would they have to account for the "felt" force or F lambda?
Under. Over it can be held still just fine. Under the event horizon of a Shwarzschild hole all things are constrained to fall toward the physical singularity. Whatever matter you have producing the normal force up on the test mass is what is responsible for that force. General relativity is not a quantum theory and as such has no gravitons. Those are proposed by particle exchange theories.
 
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  • #5
kurious said:
Is the gravitational force acting on a particle of mass m, on the
surface of a sphere of radius 10^24 metres and with a mass of
10^52 kg given by G x10^52 m / (10^24 ) ^ 1/2 - the Newtonian value - or is the mass density high enough for general relativity to be required to get a
sensible result?

The gravitational field alters the mass of the particle. If the proper mass of the particle is m0, and the particle is not moving, then the mass of the particle is

[tex]m = m_{0}\frac{dt}{d\tau} = \frac{ m_{0} }{ \sqrt{1 + 2\Phi/c^2}}[/tex]

where

[tex]\Phi = -\frac{GM}{r}[/tex]

The gravitational force G is then given by

[tex]G = \frac{GMm}{r^{2}}[/tex]

Pete
 
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  • #6
Mass is invariant. Even in the presence of a gravitational field, Riemannian spacetime curvature, the quantity
[tex]m = \frac{\sqrt{|g_{\mu }_{\nu }p^{\mu }p^{\nu }|}}{c}[/tex]
which is defined as the mass of a free particle for modern general relativity does not depend on frame, speed, position, etc. Pmb's expression is not generally covariant-
http://groups.google.com/groups?q=+...=off&selm=34EE0B44.399A3FA1@lucent.com&rnum=7
and as such is not representative of modern general relativity. On a more basic note, it is bad to use the same case of the same letter to represent two different things in the same equation as in pmb's
"[tex]G = \frac{GMm}{r^2}[/tex]"
 
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1. What is the difference between General Relativity and Newton's Laws?

General Relativity is a theory of gravity developed by Albert Einstein in the early 20th century, while Newton's Laws of Motion were developed by Sir Isaac Newton in the 17th century. General Relativity provides a more accurate and comprehensive explanation of gravity, while Newton's Laws are simpler and still accurate for most everyday situations.

2. How does General Relativity explain gravity?

General Relativity explains gravity as the curvature of spacetime caused by the presence of mass and energy. Objects with mass cause spacetime to curve, and other objects are affected by this curvature, resulting in what we perceive as gravity.

3. Are Newton's Laws still applicable in light of General Relativity?

Yes, Newton's Laws are still applicable in most everyday situations, as they provide a simpler and accurate description of motion. However, in extreme cases such as near black holes or at very high speeds, General Relativity is needed to accurately describe gravity and motion.

4. How does General Relativity impact our understanding of the universe?

General Relativity has greatly impacted our understanding of the universe by providing a better understanding of gravity and how it affects the motion of objects. It has also helped explain phenomena such as the bending of light by massive objects and the expansion of the universe.

5. Can General Relativity and Newton's Laws coexist?

Yes, they can coexist and complement each other. While General Relativity provides a more accurate and comprehensive explanation of gravity, Newton's Laws are still useful for many practical applications and are often used alongside General Relativity in modern physics.

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